The morphology and magnetic field structure of supernova remnant G93.3+6.9

Details The morphology and magnetic field structure of supernova remnant G93.3+6.9 The morphology and magnetic field structure of supernova remnant G93.3+6.9

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...131..196l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 131, no. 2, Feb. 1984, p. 196-199.

Astronomy and Astrophysics

Astrophysics

10

Astronomical Maps, Magnetic Stars, Stellar Magnetic Fields, Supernova Remnants, Depolarization, Linear Polarization, Morphology, Radio Emission

Scientific paper

Radio continuum maps at 4.75 GHz are presented of the SNR G93.3+6.9. Both total power and linear polarization observations were made. The remnant is confirmed to have a shell-type morphology and no evidence is found for the presence of significant emission from the central volume. A study of the depolarization with frequency and rotation measure has been made. It is demonstrated that the magnetic field in the shell is circumferential and well-ordered across the whole remnant.

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